Potential mechanisms for the formation of planetary crust matter

Details Potential mechanisms for the formation of planetary crust matter Potential mechanisms for the formation of planetary crust matter

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988geokh......150b&link_type=abstract

Geokhimiia (ISSN 0016-7525), Feb. 1988, p. 150-179. In Russian.

Computer Science

Computerized Simulation, Planetary Composition, Planetary Crusts, Planetary Evolution, Terrestrial Planets, Earth Crust, Earth Mantle

Scientific paper

The geochemical composition of the terrestrial planets' crust matter is described, and the possible mechanisms responsible for its formation are discussed using results obtained in earlier studies. These data, together with the information on the thermal history of planets during their evolution, are used to develop a model of planetary matter differentiation due to evaporation-condensation processes in the course of impact events during accretion. The results of a computer simulation of early magmatic differentiation of an earth-type planet are given.

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